Fundamental physics with blazar spectra: a critical appraisal

TL;DR

This paper critically evaluates how high-energy BL Lac spectra can test physics beyond the standard model, analyzing different scenarios like ALP interactions, LIV, and hadron beams, and discusses how upcoming telescopes can distinguish these models.

Contribution

It provides a comparative analysis of multiple beyond-standard-model scenarios affecting blazar spectra and suggests observational signatures to differentiate them using future telescopic data.

Findings

Photon-ALP interactions produce spectral oscillations.

LIV causes a peak around 100 TeV in spectra.

Hadron beams and ALP interactions predict extended hard tails.

Abstract

Very-high-energy (VHE) BL Lac spectra extending above $10 \, \rm TeV$ provide a unique opportunity for testing physics beyond the standard model of elementary particle and alternative blazar emission models. We consider the hadron beam, the photon to axion-like particle (ALP) conversion, and the Lorentz invariance violation (LIV) scenarios by analyzing their consequences and induced modifications to BL Lac spectra. In particular, we consider how different processes can provide similar spectral features (e.g. hard tails) and we discuss the ways they can be disentangled. We use HEGRA data of a high state of Markarian 501 and the HESS spectrum of the extreme BL Lac (EHBL) 1ES 0229+200. In addition, we consider two hypothetical EHBLs similar to 1ES 0229+200 located at redshifts $z=0.3$ and $z=0.5$. We observe that both the hadron beam and the photon-ALP oscillations predict a hard tail extending to energies larger than those possible in the standard scenario. Photon-ALP interaction predicts a peak in the spectra of distant BL Lacs at about $20-30 \, \rm TeV$, while LIV produces a strong peak in all BL Lac spectra around $\sim 100 \, \rm TeV$. The peculiar feature of the photon-ALP conversion model is the production of oscillations in the spectral energy distribution, so that its detection/absence can be exploited to distinguish among the considered models. The above mentioned features coming from the three models may be detected by the upcoming Cherenkov Telescope Array (CTA). Thus, future observations of BL Lac spectra could eventually shed light about new physics and alternative blazar emission models, driving fundamental research towards a specific direction.